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20112022
most citedKIC 3858884: a hybrid δ Sct pulsator in a highly eccentric eclipsing binary

70 citations · 89 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2022★ 5 cited

V1294 Aql = HD 184279: A bad boy among Be stars or an important clue to the Be phenomenon?

P. Harmanec, H. Božić, P. Koubský +21

A reliable determination of the basic physical properties and variability patterns of hot emission-line stars is important for understanding the Be phenomenon and ultimately, the e…

astro-ph.SR2021★ 4 cited

Long-term, orbital, and rapid variations of the Be star V923 Aql = HD 183656

M. Wolf, P. Harmanec, H. Božić +9

We present the latest results of a long-term observational project aimed at observing, collecting from the literature, and homogenising the light, colour, and spectral variations o…

astro-ph.SR2020★ 8 cited

The SDSS-HET Survey of Kepler Eclipsing Binaries. Description of the Survey and First Results

Suvrath Mahadevan, Chad F. Bender, Kelly Hambleton +9

The Kepler mission has provided a treasure trove of eclipsing binaries (EBs), observed at extremely high photometric precision, nearly continuously for several years. We are carryi…

astro-ph.SR2014★ 70 cited

KIC 3858884: a hybrid δ Sct pulsator in a highly eccentric eclipsing binary

C. Maceroni, H. Lehmann, R. da Silva +10

The analysis of eclipsing binaries containing non-radial pulsators allows: i) to combine two different and independent sources of information on the internal structure and evolutio…

astro-ph.SR2011★ 2 cited

V2368 Oph: An eclipsing and double-lined spectroscopic binary used as a photometric comparison star for U Oph

P. Harmanec, H. Božić, P. Mayer +8

The A-type star HR 6412 = V2368 Oph was used by several investigators as a photometric comparison star for the known eclipsing binary U Oph but was found to be variable by three in…